Name: X-Ray Astronomy with the Einstein Satellite: Proceedings of the High Energy Astrophysics Division of the American Astronomical Society Meeting on X-Ra (en Inglés)
Price: 506.54 PEN
Availability: InStock
Author: Giacconi, R.
ISBN: 9789400984615

portada X-Ray Astronomy with the Einstein Satellite: Proceedings of the High Energy Astrophysics Division of the American Astronomical Society Meeting on X-Ra (en Inglés)

Formato

Libro Físico

Editorial

Springer

Autor

Giacconi, R.

Idioma

Inglés

N° páginas

330

Encuadernación

Tapa Blanda

Dimensiones

23.4 x 15.6 x 1.8 cm

Peso

0.48 kg.

ISBN13

9789400984615

Categorías

Astronomía, espacio y tiempo
Jardinería
Astronomía popular y el espacio

X-Ray Astronomy with the Einstein Satellite: Proceedings of the High Energy Astrophysics Division of the American Astronomical Society Meeting on X-Ra (en Inglés)

Giacconi, R. (Autor) · Springer · Tapa Blanda

Libro Nuevo

S/ 506,54

S/ 1.013,08

Ahorras: S/ 506,54

50% descuento

Envío normal

Origen: Estados Unidos (Costos de importación incluídos en el precio)

Se enviará desde nuestra bodega entre el Miércoles 24 de Julio y el Viernes 02 de Agosto.

Lo recibirás en cualquier lugar de Perú entre 2 y 5 días hábiles luego del envío.

Reseña del libro "X-Ray Astronomy with the Einstein Satellite: Proceedings of the High Energy Astrophysics Division of the American Astronomical Society Meeting on X-Ra (en Inglés)"

The meeting of the High Energy Astrophysics Division of the American Astronomical Society, held in Cambridge, Massachusetts on January 28- 30, 1980, marks the coming of age of X-ray astronomy. In the 18 years since the discovery of the first extrasolar X-ray source, Sco X-l, the field has experienced an extremely rapid instrumentation development culminating with the launch on November 13, 1978 of the Einstein Observatory (HEAO-2) which first introduced the use of high resolution imaging telescopes to the study of galactic and extragalactic X-ray sources. The Einstein Observatory instruments can detect sources as faint as 10-7 Sco X-lor about 17 magnitudes fainter. The technological developments in the field have been paralleled by a host of new discoveries: in the early 1960's the detection of 9 "X-ray stars", objects 10 times more luminous in X-rays than the Sun and among the brightest stellar objects at all wavelengths; in the late 1960's and early 1970's the discovery of the natureof such systems which were identified as collapsed stars (neutron stars and black holes) in mass exchange binary systems, and the detection of the first few extragalactic sources.